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相关论文: Low-mass star formation in Lynds 1333

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We present first results from an HST/ACS imaging survey of stars and star clusters in five nearby spiral galaxies. This contribution concentrates on NGC 1313, a highly distorted late-type barred spiral. We compare the field star and cluster…

天体物理学 · 物理学 2009-11-13 S. S. Larsen , M. D. Mora , J. P. Brodie , T. Richtler

We report the results of a survey of low mass Class I protostars in the cm continuum. In the initial survey, seven sources in the Taurus star formation were observed with the VLA at 0``.25 resolution. All seven sources drive CO outflows and…

天体物理学 · 物理学 2015-06-24 P. W. Lucas , Katherine M. Blundell , P. F. Roche

Using the Infrared Array Camera and the Multiband Imaging Photometer aboard the {\it Spitzer Space Telescope}, we have obtained images of the Lupus 3 star-forming cloud at 3.6, 4.5, 5.8, 8.0, and 24 \micron. We present photometry in these…

天体物理学 · 物理学 2008-11-26 P. R. Allen , K. L. Luhman , P. C. Myers , S. T. Megeath , L. E. Allen , L. Hartmann , G. G. Fazio

As part of a multi-faceted program to investigate the origin and early evolution of sub-stellar objects, we present high-resolution Keck optical spectra of 14 very low mass sources in the IC 348 young cluster and the Taurus star-forming…

天体物理学 · 物理学 2009-11-07 Ray Jayawardhana , Subhanjoy Mohanty , Gibor Basri

We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope (UKIRT), of the Local Group spiral galaxy M33 (Triangulum). On the basis of their variability, we have identified stars in the very final stage of their…

We report the results of a near-infrared imaging study of a $7.8 \times 7.8$ arcmin$^2$ region centered on the 6.7 GHz methanol maser associated with the RCW 34 star forming region using the 1.4m IRSF telescope at Sutherland. A total of…

星系天体物理 · 物理学 2015-06-05 D. J. van der Walt , H. M. de Villiers , R. J. Czanik

We have carried out near-infrared spectroscopic observations of 23 very low-luminosity young stellar object (YSO) candidates and 5 their companions in Heiles Cloud 2, one of the densest parts of the Taurus molecular cloud. Twelve objects…

天体物理学 · 物理学 2015-06-24 Y. Itoh , M. Tamura , A. Tokunaga

The Taurus molecular cloud complex is the paradigm for quiescent, low-density, isolated star formation. Yet the age distribution of its stellar population indicates that star formation is a rapid and dynamic process, inconsistent with the…

天体物理学 · 物理学 2007-05-23 Lee Hartmann

We compiled and investigated the infrared/sub-mm/mm SED of the new outburst star IRAS 05436-0007 in quiescent phase. The star is a flat-spectrum source, with an estimated total luminosity of L_bol ~ 5.6 L_sun, typical of low-mass T Tauri…

天体物理学 · 物理学 2009-11-10 P. Ábrahám , Á. Kóspál , Sz. Csizmadia , A. Moór , M. Kun , G. Stringfellow

To investigate the environment of HII region Sh2-163 and search for evidence of triggered star formation in this region, we performed a multi-wavelength study of this HII region. Most of our data were taken from large-scale surveys: 2MASS,…

星系天体物理 · 物理学 2017-02-14 Naiping Yu , Jun-Jie Wang , Nan Li

We report a discovery of young stellar objects associated with a molecular cloud at the edge of the optical disk of our Galaxy. This cloud is denoted as Cloud 2 in the list by Digel et al. and it is one of the most distant molecular clouds…

天体物理学 · 物理学 2009-10-31 Naoto Kobayashi , Alan T. Tokunaga

We examine FUV images of the LITTLE THINGS sample of nearby dwarf irregular (dIrr) and Blue Compact Dwarf (BCD) galaxies to identify distinct young regions in their far outer disks. We use these data, obtained with the Galaxy Evolution…

星系天体物理 · 物理学 2016-05-25 Deidre A. Hunter , Bruce G. Elmegreen , Elizabeth Gehret

This paper describes a high-resolution, infrared spectroscopic survey of young, low-mass stars designed to identify and characterize pre-main-sequence spectroscopic binaries. This is the first large infrared radial velocity survey of very…

天体物理学 · 物理学 2008-11-26 L. Prato

This study aims to determine the main physical parameters (N(H2) hydrogen column density and Td dust temperature) of the Interstellar medium, and their distribution in the extended star-forming region, which includes IRAS 05156+3643,…

星系天体物理 · 物理学 2021-12-08 E. H. Nikoghosyan , N. M. Azatyan , D. H. Andreasyan , D. S. Baghdasaryan

We present a new method to derive 2D star formation histories in dwarf irregular galaxies. Based on multicolor stellar photometry data we have found that in the Leo A galaxy during the last $\sim$400 Myr star formation was propagating…

星系天体物理 · 物理学 2019-11-06 Marius Čeponis , Rima Stonkutė , Vladas Vansevičius

We present the analysis of 16 classical T Taur stars using LAMOST and TESS data, investigating spectral properties, photometric variations, and mass-accretion rates. All 16 stars exhibit emissions in H$\alpha$ lines, from which the average…

太阳与恒星天体物理 · 物理学 2023-08-03 Chia-Lung Lin , Wing-Huen Ip , Yao Hsiao , Tzu-Hueng Chang , Yi-han Song , A-Li Luo

We present VRI photometry of 320,917 stars with 11 < R < 18 throughout the lambda Orionis star-forming region. We statistically remove the field stars and identify a representative PMS population throughout the interior of the molecular…

天体物理学 · 物理学 2009-11-07 Christopher J. Dolan , Robert D. Mathieu

We summarize Hubble Space Telescope (HST) UV observations of the weak-lined T Tauri star (wTTS) PDS 70 obtained with the Space Telescope Imaging Spectrograph (STIS). These observations provide the first far-UV (FUV) and near-UV (NUV)…

太阳与恒星天体物理 · 物理学 2022-10-26 Stephen L. Skinner , Marc Audard

Does star formation proceed in the same way in large spirals such as the Milky Way and in smaller chemically younger galaxies? Earlier work suggests a more rapid transformation of H$_2$ into stars in these objects but (1) a doubt remains…

星系天体物理 · 物理学 2016-04-20 Jonathan Braine , Pierre Gratier , Carsten Kramer , Karl F. Schuster , Fatemeh Tabatabaei , Erwan Gardan

Six young bipolar outflows in regions of low-to-intermediate-mass star formation were observed in the 7_0-6_1A+, 8_0-7_1A+, and 5_{-1}-4_0E methanol lines at 44, 95, and 84 GHz, respectively. Narrow features were detected towards NGC…

天体物理学 · 物理学 2009-11-11 S. V. Kalenskii , V. G. Promyslov , V. I. Slysh , P. Bergman , A. Winnberg
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